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The dark bands are caused from the differnet chemical elements which absorb light at specific wavelengths.

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How does atomic spectrum differ from solar spectrum?

Atomic spectrum is produced when atoms emit or absorb light at specific energies, creating distinct lines or bands. Solar spectrum is the continuous spectrum of light emitted by the Sun, containing all wavelengths of light. Solar spectrum is produced by many elements and compounds in the Sun's atmosphere, creating a broad, continuous range of colors.


How is the solar system observed?

It Depends on What You Mean , But The Solar System is Observed with a Telescope.


What has the author Marc S Allen written?

Marc S. Allen has written: 'High resolution atlas of the solar spectrum 2678-2831 A' -- subject- s -: Charts, diagrams, Solar Spectrum, Spectrum, Solar, Spectrum, Ultraviolet, Ultraviolet Spectrum


What has the author Charles Edward St John written?

Charles Edward St. John has written: 'Revision of Rowland's Preliminary table of solar spectrum wave-lengths' -- subject(s): Solar Spectrum, Spectrum analysis, Spectrum, Solar


What has the author J Houtgast written?

J. Houtgast has written: 'The variations in the profiles of strong Fraunhofer lines along a radius of the solar disc' -- subject(s): Solar Spectrum, Spectrum analysis, Spectrum, Solar


What were dark lines in the spectrum named for?

Dark lines in the spectrum were named after German physicist Joseph von Fraunhofer, who first systematically studied them. They are commonly known as Fraunhofer lines and are formed when certain chemical elements absorb specific wavelengths of light, creating dark bands in the spectrum.


How did Sir Norman Lockyer discover helium?

Sir Norman Lockyer discovered helium in 1868 in the spectrum of the sun during a solar eclipse. He noticed a yellow line in the sun's spectrum that did not correspond to any known element at the time, leading to the discovery of the new element helium.


What kind of spectrum is a solar spectrum?

the answer to this question is when you use the power around you and it comes in as one so basically that is why it is called solar power


How are fraunhofer lines observed?

Fraunhofer lines are observed in the solar spectrum by using a spectroscope to disperse sunlight into its component colors. These dark absorption lines are caused by the absorption of specific wavelengths of light by elements in the Sun's atmosphere. By studying the positions and intensities of these lines, scientists can learn about the composition and physical properties of the Sun.


What has the author Fredrick N Veio written?

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When there is a lunar eclipse observed from earth what eclipse will be observed from moon?

During a lunar eclipse observed from Earth, a solar eclipse would be observed from the perspective of the Moon. This occurs because the Earth blocks the sunlight from directly reaching the Moon, resulting in a solar eclipse from the Moon's point of view.


Where did the name of the element helium come from?

It comes from the Greek word "helios" meaning "sun" after Pierre-Jules-César Janssen observed a new yellow line (587.49 nm) in the solar spectrum of the solar eclipse of 1868.